What is the mass limit above which the self-gravity of stars can overcome electron degeneracy pressure?

Question

Quizplus · Accepted Answer

The mass limit above which the self-gravity of stars can overcome electron degeneracy pressure is called the Chandrasekhar limit, which is approximately 1.4 times the mass of the Sun (1.4 Mε). If a star's mass exceeds this limit, the core of the star will collapse further, leading to a Type Ia supernova.

What Is the Mass Limit Above Which the Self-Gravity of Stars